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Quaternary variability of Indian Ocean monsoon winds and climate.

机译:印度洋季风和气候的第四纪变化。

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摘要

Satellite and meteorological observations, aerosol measurements, sediment trap studies, and studies of the mineralogical distribution of surface sediments, indicate an eolian transport mechanism for the lithogenic component of modern Arabian Sea sediments. Sediment cores from the Owen Ridge, northwest Arabian Sea, indicate that an eolian transport mechanism predominated over the past one million years. Spectral comparison of the lithogenic grain size and flux records, in addition to comparisons with independent eolian records, indicate that the grain size record can be used as a paleoclimatic indicator of summer monsoon wind strength and the flux record as an indicator of aridity in the dust source-areas (primarily the Somali and Arabian Peninsulas).;The flux record is spectrally coherent and in phase the marine oxygen isotope record over all of the Earth's primary orbital frequencies (eccentricity, obliquity, and precession). This indicates that the timing of increases and decreases in regional aridity can be explained by the interplay between orbitally-induced insolation changes and the time constant of terrestrial ice sheets.;Spectral analyses of the grain size record indicates that the strength and timing of the paleomonsoon are forced externally by changes in insolation associated with the Earth's orbital precession and internally by the availability of latent heat collected over the Indian Ocean and released over the Asian Plateau. In contrast, sensitivity tests indicate that global climate model (GCM) paleomonsoon winds respond primarily to glacial boundary conditions and secondarily to insolation changes. Such discrepancies are clearly evident in comparison of results from GCM paleomonsoon simulations with the grain size record of monsoon wind strength and with faunal estimates of wind-induced upwelling in the Arabian Sea. These findings suggest the need for sensitivity experiments examining the role of latent heat exchange in current GCM's and for continued evaluation of methods for the model parameterization of energy exchanges across the ocean-atmosphere boundary.
机译:卫星和气象观测,气溶胶测量,沉积物陷阱研究以及对表面沉积物矿物学分布的研究表明,现代阿拉伯海沉积物的成岩成分是风成岩的传输机制。来自阿拉伯海西北部欧文岭的沉积物岩心表明,在过去的一百万年中,风成岩的运输机制占主导地位。岩石成因粒度和通量记录的光谱比较,以及与独立风成记录的比较表明,该粒度记录可以用作夏季风风强度的古气候指标,通量记录可以用作粉尘干旱的指标流量记录在光谱上是相干的,并且在地球所有主要轨道频率(偏心率,倾角和进动)上海洋氧同位素的记录都是相干的。这表明区域干旱的增加和减少的时机可以用轨道诱发的日照变化与陆地冰盖的时间常数之间的相互作用来解释。;对粒度记录的频谱分析表明,古季风的强度和时机它们是由与地球轨道进动相关的日射变化而在外部产生的,而在印度内部则是由于在印度洋上收集并在亚洲高原上释放的潜热的存在而被迫产生的。相反,敏感性测试表明,全球气候模式(GCM)古季风主要对冰川边界条件做出响应,其次对日照变化做出响应。通过GCM古季风模拟的结果与季风风强度的粒度记录以及阿拉伯海中风诱发的上升流的动物学估计相比,这种差异显而易见。这些发现表明需要进行敏感性实验,以检查潜热交换在当前GCM中的作用,并需要继续评估跨海洋-大气边界的能量交换模型参数化方法。

著录项

  • 作者

    Clemens, Steven Curtis.;

  • 作者单位

    Brown University.;

  • 授予单位 Brown University.;
  • 学科 Geology.;Physical oceanography.;Paleoecology.;Ocean engineering.
  • 学位 Ph.D.
  • 年度 1990
  • 页码 332 p.
  • 总页数 332
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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